2021
DOI: 10.1098/rsos.211166
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Requirements for a global lidar system: spaceborne lidar with wall-to-wall coverage

Abstract: Lidar is the optimum technology for measuring bare-Earth elevation beneath, and the structure of, vegetation. Consequently, airborne laser scanning (ALS) is widely employed for use in a range of applications. However, ALS is not available globally nor frequently updated due to its high cost per unit area. Spaceborne lidar can map globally but energy requirements limit existing spaceborne lidars to sparse sampling missions, unsuitable for many common ALS applications. This paper derives the equations to calcula… Show more

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Cited by 33 publications
(22 citation statements)
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“…The swath width of a spaceborne lidar can be calculated by considering the lidar performance and the spacecraft orbital velocity. The lidar equation can be combined with the orbital velocity equation to express the swath width as a function of orbit altitude as [18] where s is the swath width, P pay is the power available to the lidar payload from the spacecraft bus, L e is the laser efficiency, E det is the energy detected at the receiver (after detector efficiency losses), A is the telescope collecting area, h is the orbit altitude, is the atmospheric transmittance, Q is the detector quantum efficiency, is the surface reflectance, R is the mean Earth radius, r is the desired spatial resolution of the instrument, and is the standard gravitational parameter of Earth. A full derivation of equation ( 1) is provided in [18].…”
Section: Swath Widthmentioning
confidence: 99%
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“…The swath width of a spaceborne lidar can be calculated by considering the lidar performance and the spacecraft orbital velocity. The lidar equation can be combined with the orbital velocity equation to express the swath width as a function of orbit altitude as [18] where s is the swath width, P pay is the power available to the lidar payload from the spacecraft bus, L e is the laser efficiency, E det is the energy detected at the receiver (after detector efficiency losses), A is the telescope collecting area, h is the orbit altitude, is the atmospheric transmittance, Q is the detector quantum efficiency, is the surface reflectance, R is the mean Earth radius, r is the desired spatial resolution of the instrument, and is the standard gravitational parameter of Earth. A full derivation of equation ( 1) is provided in [18].…”
Section: Swath Widthmentioning
confidence: 99%
“…To avoid this, a minimum resolution limit ( r min ) is defined that will ensure that a continuous track at least one pixel wide with E det per shot can be produced. This is detailed in [18] and can be calculated by using equation (1) and letting s = r = r min , giving (4)…”
Section: Resolutionmentioning
confidence: 99%
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